Noble Dark Matter: Surprising Elusiveness of Dark Baryons

TL;DR

This paper explores a class of dark matter models where dark baryons, transforming under SU(2)$_L$, are predominantly singlets at TeV scales, making them elusive and akin to noble gases, thus challenging detection efforts.

Contribution

It classifies dark baryon states in confining SU(2)$_L$ sectors, calculates their mass spectra, and introduces the concept of Noble Dark Matter as inert, singlet-dominant states.

Findings

Dark baryons are mostly singlets at TeV scales.

Singlet nature suppresses interactions with Standard Model.

Noble Dark Matter resembles inert noble gases.

Abstract

Dark matter could be a baryonic composite of strongly-coupled constituents transforming under SU(2)$_L$. We classify the SU(2)$_L$ representations of baryons in a class of simple confining dark sectors and find that the lightest state can be a pure singlet or a singlet that mixes with other neutral components of SU(2)$_L$ representations, which strongly suppresses the dark matter candidate's interactions with the Standard Model. We focus on models with a confining $\text{SU}(N_c)$ and heavy dark quarks constituting vector-like $N_f$-plet of SU(2)$_L$. For benchmark $N_c$ and $N_f$, we calculate baryon mass spectra, incorporating electroweak gauge boson exchange in the non-relativistic quark model, and demonstrate that above TeV mass scales, dark matter is dominantly a singlet state. The combination of this singlet nature with the recently discovered $\mathcal{H}$-parity results in an inert state analogous to noble gases, hence we coin the term Noble Dark Matter. Our results can be understood in the non-relativistic effective theory that treats the dark baryons as elementary states, where we find singlets accompanying triplets, 5-plets, or more exotic representations. This generalization of WIMP-like theories is more difficult to find or rule out than dark matter models that include only a single SU(2)$_L$ multiplet (such as a Wino), motivating new searches in colliders and a re-analysis of direct and indirect detection prospects in astrophysical observations.